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On the exceptional set of Lagrange’s equation with three prime and one almost–prime variables

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(1)

On the exceptional set of Lagrange’s equation

with three prime and

one

almost-prime variables

par DOYCHIN TOLEV

RÉSUMÉ. Nous considérons une version affaiblie de la conjecture

sur la représentation des entiers comme somme de quatre carrés de nombres premiers.

ABSTRACT. We consider an approximation to the

popular

con- jecture about representations of integers as sums of four squares of prime numbers.

1. Introduction and statement of the result

The famous theorem of

Lagrange

states that every

non-negative integer

n can be

represented

as

where ~i,...,.r4 are

integers.

There is a

conjecture,

which asserts that

every

sufficiently large integer

n, such that n - 4

(mod 24~,

can be repre-

sented in the form

(1.1)

with

prime

variables ~1, .. , x4. This

conjecture

has not been

proved

so

far,

but there are various

approximations

to it

established.

We have to mention first that in 1938 Hua

[9] proved

the

solvability

of

the

corresponding equation

with five

prime

variables. In 1976 Greaves

[3]

and later Shields

[19]

and Plaksin

[18] proved

the

solvability

of

(1.1)

with

two

prime

and two

integer

variables

(in [18]

and

[19]

an

asymptotic

formula

for the number of solutions was

found).

In 1994 Brfdern and

Fouvry [2]

considered

(1.1)

with

almost-prime

vari-

ables and

proved

that if rt is

large enough

and satisfies n - 4

(mod 24)

then

(l.l)

has solutions in

integers

of

type P34.

Here and later we denote

by P r

any

integer

with no more than r

prime factors,

counted

according

to

multiplicity. Recently

Heath-Brown and the author

[8] proved that,

under

the same conditions on rt, the

equation (l.l)

has solutions in one

prime

and

three

P101 - almost-prime

variables and also in four

P25 - almost-prime

variables. These results were

sharpened slightly by

the author

~21~,

who

lB/Ianuscrit reçu le 7janvier 2004.

(2)

established the

solvability

of

(1.1)

in one

prime

and three

P80 -

almost-

primes and, respectively,

in four

P21 - almost-primes.

There are several papers,

published during

the last years, devoted to

the

study

of the

exceptional

set of the

equation (1.1)

with

prime

variables.

Suppose

that Y is a

large

real number and denote

by El (Y)

the number

of

positive integers

n Y

satisfying

n - 4

(mod 24)

and which cannot

be

represented

in the form

(1.1)

with

prime

variables ~1, ... , ~4. In 2000

J.Liu and M.-C. Liu

[16] proved

that

y13/15+é,

where e > 0 is

arbitrarily

small. This result was

improved considerably by Wooley [22],

who established that

El(Y)

«

y13/30+é. Recently

L. Liu

[15]

established that

El (Y)

«

y2/5+é.

In the paper

[22] Wooley

obtained otller

interesting results, concerning

the

equation (1.1).

We shall state one of them. Denote

by R(n)

the number

of solutions of

(1.1)

in three

prime

and one

integer

variables. It is

expected

that

R(n)

can be

approximated by

the

where

C~(n)

is the

corresponding singular

series

(see [22]

for the

definition).

Wooley proved

that the set of

integers

n, for which

R(n)

fails to be close

to the

expected value,

is

remarkably

thin. More

precisely,

let

0(t)

be any

monotonically increasing

and

tending

to

infinity

function of the

positive

variable

t,

such that «

(logt)B

for some constant B > 0. Let Y be a

large

real number and denote

by

the number of

positive integers

Y such that

Theorem 1.2 of

[22]

asserts that

We note that if the

integer n

satisfies

Therefore,

if

E2(Y)

denotes the number of

positive integers n Y,

satis-

fying (1.2)

and which cannot be

represented

in the form

(1.1)

with three

prime

and one

integer variables,

then

for any é > 0.

The purpose of the

present

paper is to obtain an estimate of almost the

same

strength

as

(1.3)

for the

exceptional

set of the

equation (1.1)

with

three

prime

and one

almost-prime

variables. We shall prove the

following

(3)

Theorem. Let Y be a

large

real number and denote

by E(Y)

the number

of positive integers

n Y

satisfying

n - 4

(mod 24)

and which cannot be

represented

in the

form

where P1,P2,P3 are

primes

and x =

P11.

Then we have

As one may

expect,

the

proof

of this result is

technically

more

compli-

cated than the

proof

of Theorem 1.2 of

[22].

We use a combination of the circle method and the sieve methods.

In the circle method

part

we

apply

the

approach of Wooley [22], adapted

for our needs. On the set of minor arcs we

apply

the method of Klooster-

man, introduced in the classical paper

[14].

This

technique

was,

actually,

applied

also

by Wooley

in the estimation of the sums

Ti

and

T2

in section 3 of

[22].

In his

analysis, however, only Ramanujan’s

sums appear, whiles in

our situation we have to deal with much more

complicated

sums, defined

by (8.19). Fortunately,

these sums differ very

slightly

from sums considered

by

Brfdern and

Fouvry [2],

so we can, in

fact,

borrow their result for our needs.

The sieve method

part

is rather standard. We

apply

a

weighted

sieve

with

weights

of Richert’s type and

proceed

as in

chapter

9 of Halberstam

and Richert’s book

[4].

In many

places

we omit the calculations because

they

are similar to those

in other books or papers, or because

they

are standard and

straightforward.

We note that one can obtain

slightly stronger

result

(with

smaller power in

(1.5)

and with variable x

having

fewer

prime factors) by

means of more

elaborate

computational

work.

Acknowledgement.

The main part of this paper was written

during

the

visit of the author to the Institute of Mathematics of the

University

of

Tsukuba. The author would like to thank the

Japan Society

of Promotion

of Science for the financial support and to the staff of the Institute for the excellent

working

conditions. The author is

especially grateful

to Professor

Hiroshi Mikawa for the

interesting

discussions and valuable comments.

The author would like to thank also Professor Trevor

Wooley

for inform-

ing

about his paper

[22]

and

providing

with the

manuscript.

2. Notations and some definitions

Throughout

the paper we use standard number-theoretic notations. As

usual, p(n)

denotes the M6bius

function,

is the Euler

function,

is the number of

prime

divisors of n, counted

according

to

multiplicity,

(4)

T(n)

is the number of

positive

divisors of n. The

greatest

common divisor

and, respectively,

the least common

multiple

of the

integers

MI, M2 are

denoted

by (m1, m2)

and

[m1, m2]. However,

if u and v are real numbers then

(u, v)

means the interval with

endpoints u

and v. The

meaning

is

always

clear from the context. We use bold

style

letters to denote four-

dimensional vectors. The letter p is reserved for

prime

numbers.

If p

> 2

then -

stands for the

Legendre symbol.

To denote summation over the

positive integers

n Z we write

Furthermore, ~x(~,), respectively,

¿x(q)*

means that x runs over a

complete, respectively,

reduced

system

of residues modulo q.

By ~a~

we denote the

integer part

of the real number a,

e(~) - e"?"

and

eq(a)

=

e(a/q).

We assume that E > 0 is an

arbitrarily

small

positive

number and A

is an

arbitrarily large number; they

can take different values in different formulas. Unless it is not

specified explicitly,

the constants in the 0 -

terms and « -

symbols depend

on E and A. For

positive

U and V we write

!7 x V as an abbreviation of U « V « U.

Let N be a

suffciently large

real number. We define

where E > 1 is a

large

constant, which we shall

specify

later.

To

apply

the sieve method we need information about the number of solutions of

(1.4)

in

integers

x

lying

in arithmetical

progressions

and in

primes

pl, p2, p3. For technical reasons we attach

logarithmic weights

to

the

primes

and a smooth

weight

to the variable x. More

precisely,

we

consider the function

and let

For any

integer n

E

(N/2, N]

and for any

squarefree integer k,

such that

(k, 6)

=

1,

we define

We expect that this

quantity

can be

approximated,

at least on average,

by

the

expression

(5)

which arises as a mean term when we

apply formally

the circle method.

The

quantity K(n)

from the

right-hand

side of

(2.6)

comes from the

singular integral

and is defined

by

Having

in mind

(2.3)

we see that

Furthermore, 6 (n, ~;)

comes from the

singular

series and is defined

by

where

We shall consider

C‘~(7t, k)

in detail in the next section.

3. Some

properties

of the sum

6(n, k)

It is not difficult to see that the function

f (q, n,1~),

defined

by (2.10),

is

multiplicative

with

respect

to q. We shall

compute

it for q =

p~.

From this

point

onwards we assume that the

integers

n and k

satisfy

Then we have

Furthermore, if p

> 2 is a

prime,

then

(6)

and

where the

quantities hj

are defined

by

The

proof

of formulas

(3.2) - (3.8)

is standard and uses

only

the basic

properties

of the Gauss sums

(see

Hua

[10], chapter 7,

for

example).

We

leave the verification to the reader.

From

(3.2) - (3.8)

we

easily get

This estimate

implies

that the series

(2.9)

is

absolutely convergent.

We

apply

Euler’s

identity

and we use

(3.1) - (3.5)

to obtain

From this formula and

(3.4),

after some

rearrangements,

we

get

where

(7)

and where

From

(3.1), (3.5) - (3.8), (3.11)

and

(3.13)

we obtain the estimates

and

where the constant in the 0 -term in the last formula is absolute. We leave the easy verification of formulas

(3.14) - (3.17)

to the reader.

Let us note that from

(3.10), (3.12)

and

(3.16)

it follows

which we, of course,

expect, having

in mind the definition

(2.5)

of

I(n, k)

and the conditions

(3.1).

4. Proof of the Theorem

A central role in the

proof

of the Theorem

plays

the

following Proposi- tion,

which asserts that the difference between the

quantities I(n, k)

and

E(n, ~ ),

defined

by (2.5)

and

(2.6),

is small on average with

respect

to n

and k.

Proposition. Suppose

that the set F consists

of integers

n E

(N/2, N],

satisfying

the congruence n - 4

(mod 24),

and denote

by

F the

cardinality of

~’. Let

q(k)

be a real valued

function, defined

on the set

of positive integers

and such that

and

Suppose

also that

for

some constant

(8)

and conszder the sum

Then we have

The constant in

Vinogradov’s symbol depends only

on the constants

6, E, included, respectively,

in

(2.1), (2.2)

and

(4.3).

We shall prove the

Proposition

in sections 5 - 8. In this section we shall

use it to establish the Theorem.

Let ,~’ be the set of

integers n

E

(N/2, N] satisfying

n - 4

(mod 24)

and

which cannot be

represented

in the form

(1.4)

with

primes

Pi, P2, P3 and with r =

P11.

Let F be the

cardinality

of .~. We shall establish that

Obviously,

this

implies

the estimate

( 1.5) .

To

study

the

equation (1.4)

with an

almost-prime

variable x we

apply

a

weighted

sieve of Richert’s

type.

Let q, v,

vl, 9

be constants such that

Denote

and

Consider the sum

where

It is clear that

(9)

where

T1

is the contribution of the terms for which > 0. We decom- pose

f1

as

(4.13)

where

F2

is the contribution of the terms with x == 0

(mod p2)

for some

prime

p E

[z, zl)

and where

F3

comes from the other terms.

We note that the congruence condition n - 4

(mod 24)

and the size

conditions on pi in the domain of summation in

(4.10) imply

that there

are no terms with

(6, x)

> 1 counted in T

and, respectively,

in

r3.

Hence

the condition

(~, P)

= 1 from the domain of summation in

(4.10)

can be

replaced by (x. 6P)

= 1.

Furthermore,

if r is

squarefree

with respect to the

prime

numbers p E

[z, zi),

if

(~, 6P)

= 1 and

A(r)

>

0,

then

For

explanation

we refer the reader to Halberstam and Richert

[4], chap-

ter

9, p.256.

From this

point

onwards we assume also that

Then

using (4.14), (4.15)

and the definition of the set 17 we conclude that the sum

F3

is

empty,

i.e.

Indeed,

if this were not true, then for some n E .~ the

equation (1.4)

would

have a solution P1,P2,P3, x with x

satisfying (4.14). However,

this is not

possible

due to

(4.15)

and the definition of T.

It is easy to estimate

F2

from above. We have

and, having

in mind

(4.7)

and

(4.8),

we

get

From

(4.12), (4.13), (4.16)

and

(4.17)

it follows that

(10)

We shall now estimate T from below.

Using (4.10)

and

(4.11)

we repre-

sent it in the form

where

and where

F5

comes from the second term in the

right-hand

side of

(4.11).

Changing

the order of summation we

get

To find a non-trivial lower bound for r we have to estimate

r4

from below and

r5

from above. We shall

apply

Rosser’s sieve

(see

Iwaniec

[12], [13]).

First we

get

rid of the condition

(x, P)

= 1 from the domains of summa-

tion in

(4.20)

and

(4.21) by introducing

the

weight

Denote

by ~-(d)

the lower Rosser function of order D and for each

prime

p E

[z, zl)

denote

by A) (d)

the upper Rosser function of order

D/p. They satisfy

and

(11)

Furthermore,

let

f (s)

and

F(s)

be the functions of the linear sieve. We consider

separately

the cases

5 I nand 5 f n

and use

(3.15) - (3.17), (4.7) -

(4.9)

to find that

where

For the definition and

properties

of Rosser’s functions and the functions

f (s), F(s)

as well as for

explanation

of

(4.23) - (4.27)

we refer the reader

to Iwaniec

[12], ~13~.

Consider the sum

F4.

From

(2.5), (4.20), (4.22), (4.23)

and

(4.25)

we get

where

and where

Consider now

F5 - Using (4.21), (4.22)

and

(4.25)

we find that

where

r7

comes from the

quantity

from the

right-hand

side of

(4.25).

Changing

the order of summation and

applying (2.5), (4.9)

and

(4.24)

we

write

IF7

in the form

(12)

where

Using (4.8), (4.9), (4.23), (4.24), (4.30)

and

(4.32)

we see that both func-

tions

q’(k)

and

q"(k) satisfy

the conditions

(4.1)

and

(4.2).

We consider the sums

and

using

the

Proposition

we conclude that

According

to

(4.19), (4.29), (4.31)

and

(4.34)

we have

Consider more

precisely

the sums

F8

and

r9.

From

(2.6), (3.10), (3.18), (4.30)

and

(4.33)

it follows that

and, respectively,

we

apply (2.6), (3.10), (3.18)

and

(4.33)

to

get

Furthermore, according

to

(3.12), (4.24)

and

(4.32)

we have

From

(2.8), (3.14) - (3.17), (4.26) - (4.28)

and

(4.36) - (4.38)

we obtain

where

(13)

Now we

apply

the

arguments

of Halberstam and Richert

~4~, chapter 9,

p. 246 and we find

where

We

specify

the constants included

by

It is easy to see that

they satisfy

the conditions

(4.7)

and

(4.15).

Further-

more,

using

Lemma 9.1 of Halberstam and Richert

[4],

we can

verify

that

if q, v, vl and 0 are

specified by (4.41),

then

From

(2.8), (3.14), (4.28), (4.39), (4.40)

and

(4.42)

we

get

where Co > 0 is a constant.

Inequalities (4.18), (4.35)

and

(4.43) imply

We are now in a

position

to

apply

the main idea of

Wooley ~22~.

Since

E > 1 we can omit the second term from the

right-hand

side of

(4.44).

We

get

which

implies

the estimate

(4.6)

and proves the Theorem.

5. The

proof

of the

Proposition

-

beginning

We represent the sum

I(n, k;),

defined

by (2.5),

in the form

where

The

integration

in

(5.1)

can be taken over any interval of

length

one

and,

in

particular,

over

, _ _ "1 - - " .

(14)

We

represent Jo

as an union of

disjoint Farey

intervals

where

and where

q’

and

q"

are

specified by

the conditions

(5.4)

X

q + q’, q + q" aq’ ==

1

(mod q) , aq" - -1 (mod q) (for

more details we refer the

reader,

for

example,

to

Hardy

and

Wright [5], chapter 7).

Consider the set

where

It is clear that if

1 a q P, (a, q)

=

1,

then

91(q, a)

c

B(q, a),

hence

we can represent

Jo

in the form

where

Hence we have

where

From

(4.4), (5.10)

and

(5.11)

we see that the sum E can be

represented

as

(15)

where

To prove the

Proposition

we have to estimate the sums

£1 and £2.

We shall

consider

£1

in section 6 and

£2 -

in sections 7 and 8.

6. The estimation of the sum

~l

We

apply

Lemma 3.1

of Wooley [22],

which is based on the earlier result of

Bauer,

Liu and Zhan

[1].

It states that if the set .M is defined

by (5.5),

then for any

integer h

such that 1 h

N,

we have

where

Using (5.2)

and

(5.11)

we write

7i

in the form

We now

apply (2.3), (2.4)

and

(6.1)

to

get

11B I t,,,

where

We note

that,

due to the choice of our

weight w(x),

it is not necessary to consider

analogs

of formula

(6.1)

for

non-positive integers h,

as it was done

in

[22].

Using (4.2), (5.13)

and

(6.3)

we find

(16)

where

Consider first

£i2).

* It was established in

[22]

that

so,

using (2.1), (6.5), (6.7)

and

(6.8)

we find

where

It is clear that

Applying

Theorem 3 of Hua

[11]

we find

for some absolute constant B > 0. From

(6.9)

and

(6.10)

we conclude that

if E > B +

1,

which we shall assume, then

Consider now the sum

£i1).

First we

apply (6.2)

and

(6.4)

to write the

expression l(l)

in the form

where

Furthermore,

we have

(17)

where

Obviously,

if

(k, q) t

m, then W* = 0. If

(k, q) I

m, then there exists

unique h

=

(mod [k, q]),

such that the

system

of congruences in the domain of summation of

(6.14)

is

equivalent

to r m h

(mod [k, q]).

We

apply

Poisson’s summation formula and use

(2.3)

and

(2.4).

After some

calculations we

get

1 then we

integrate

the last

integral by

parts m times.

Having

in

mind the conditions k

D, q

P and

using (2.1)

and

(4.3)

we find that

the

integral

is

where the constant in

Vinogradov’s symbol depends only

on m. From this

observation we conclude that the contribution to

W*, coming

from the

terms

1,

is

negligible.

More

precisely,

we have

where

K(n)

is defined

by (2.7)

and where the constant A > 0 is

arbitrarily large.

From

(2.10), (2.11), (6.12), (6.13)

and

(6.15)

we

get

It remains to take into account also

(2.6), (2.8), (2.9)

and

(3.9)

and we find

This formula and

(2.1), (4.2), (6.7) imply

We note that any,

arbitrarily

small

positive

value of the constant 6 from the definition of

P,

suffices for the

proof

of the last estimate. This

happens

wherever P occurs, so any progress in

obtaining asymptotic

formulas of

type (6.1)

for

larger

sets of

major

arcs is not relevant to our

problem.

Finally,

from

(6.6), (6.11)

and

(6.16)

we obtain the estimate

(18)

7. The estimation of the sum

62

Using (5.11)

and

(5.13)

we

represent

the sum

92

in the form

where

Applying

H61der’s

inequality

we

get

where

For

T1

we

apply

the well known estimate

,,1

Consider

Tz.

From

(7.1)

and

(7.3)

we

get

where

To estimate the first term from the last line of

(7.5)

we

apply

the in-

equality

Its

proof

is very similar to the

proof

of formula

(4.3)

from author’s pa- per

[20],

so we omit it.

(19)

In the next section we shall estimate

~(l)

and we shall prove that

From

(2.1), (4.3), (7.5), (7.7)

and

(7.8)

we obtain

Applying (7.2), (7.4)

and

(7.9)

we

get

It remains to combine

(5.12), (6.17)

and

(7.10)

and we find that the estimate

(4.5) holds,

which proves the

Proposition.

8. The estimation of

For any

integers

a, q,

satisfying 1 a q X, (a, q)

=

1,

we consider

the set

9R(q, a),

defined

by

where the

integers q’

and

q"

are

specified by (5.4). Using (5.3), (5.6), (5.8), (5.9), (7.6)

and

(8.1)

we find that

X,

then we have

where

Formula

(8.3)

is a

special

case of Lemma 12 from the paper

[8] by

Heath-

Brown and the author.

(20)

From

(7.1)

and

(8.3)

it follows that the

integrand

in

(8.2)

can be repre-

sented in the form

where

and where n, k and u are four dimensional vectors with

components,

re-

spectively,

ni,

ki

and ui, i =

1, 2, 3, 4.

We substitute the

expression (8.6)

for the

integrand

in

(8.2). Then,

in

order to

apply

Kloosterman’s

method,

we

change

the order of

integration

and summation over a. We find that

where

To

proceed

further we have to express the condition

a) 3 /3

in more

convenient form. We do this in a standard way

by introducing

a function

Q(v,

q,

~3),

defined for

integers

q, v such that 1 q

X, -q/2

v

q/2

and real numbers

{3

E

[_(qX)-l, (qX)-l].

For fixed v and q this function is

integrable

with respect to

/3

and

satisfy

(21)

Furthermore,

if

(a, q)

=

1,

if a

(mod q)

is defined

by

aa - 1

(mod q)

and

if q’ and q"

are

specified by (5.4),

then

A construction of a function with these

properties

is

available,

for

example,

in Heath-Brown

[7],

section 3.

Using (8.13)

we can express the condition

a) 3 j3

from the domain

of summation in

(8.10).

If P

q X, then, according

to

(8.1), (8.11)

and

(8.13),

we find that

N

If q

P then we

integrate

over

hence, having

in mind

(8.1),

we see that the condition

OO1(q, a) 3 /3

in

(8.10)

is

equivalent

to

(

2013

., ..] 1

3

0.

Therefore we can use

again (8-13)

is

equivalent {3.

Therefore we can use

again (8.13)

to obtain

(8.14).

We conclude that

~(l)

can be written in the form

where

Using (4.1), (4.2), (8.12)

and

(8.15)

we find that

, ,- ,

where

E’

means that the summation is taken over

squarefree odd ki

and

(22)

Consider the sum W. From

(8.4), (8.8)

and

(8.16)

we see that it can be

written as

In this form the sum W is very similar to a sum, considered

by

Brfdern

and

Fouvry [2]. Applying

the

method, developed

for the

proof

of Lemma 1

from

[2],

we find that if

~2

are

squarefree

odd

integers,

then

Consider the

quantity T,

defined

by (8.18). Obviously

Applying (8.5), (8.7), (8.9), (8.21)

and Lemma

10(ii)

of

[8]

we

get

If n = 0 and P

q X,

then we use

(8.5), (8.9), (8.21)

and

apply

the

well known estimate

We

get

If n = 0 and q

P,

then we use

(2.2), (8.11), (8.18)

and

(8.23)

to obtain

From

(8.17)

we find that

where is the contribution of the terms from the

right-hand

side of

(8.17)

such that

n ~ 0, ’b2

comes from the terms with n = 0 and P

q ~

X

and, finally, ~3

comes from the terms for which n = 0

and q

P.

(23)

To estimate we use

(8.20)

and

(8.22)

and we

get

After some standard

calculations,

which are very similar to those in sec-

tion 5 of

[8],

we obtain

We leave the verification of this estimate to the reader.

For

~2

we

apply (8.20)

and

(8.24)

to

get

To estimate

Q3

we

apply, respectively, (8.20)

and

(8.25)

and we find

, - , ’I. , - , .

The estimate

(7.8)

is a consequence of

(8.26) - (8.29).

This proves the

Proposition

and now the

proof

of the Theorem is com-

plete.

Added in

proof:

Two

interesting results, concerning

the

quantity E1 (Y),

defined in section

1, appeared

since the present paper was submitted for

publication. J.Liu, Wooley

and Yu

[17]

established the estimate

E1 (Y)

«

Y’18+6

and very

recently

Harman and Kumchev

[6] proved

that

El (Y)

GC

References

[1] C. BAUER. M.-C. LIU. T. ZHAN, On a sum of three prime squares. J. Number Theory 85 (2000), 336-359.

[2] J. BRÜDERN. E. FOUVRY, Lagrange’s Four Squares Theorem with almost prime variables.

J. Reine Angew. Math. 454 (1994), 59-96.

[3] G. GREAVES, On the representation of a number in the form x2 + y2 + p2 + q2 where p and q are odd primes. Acta Arith. 29 (1976), 257-274.

[4] H. HALBERSTAM. H.-E. RICHERT, Sieve methods. Academic Press, 1974.

[5] G. H. HARDY. E. M. WRIGHT, An introduction to the theory of numbers. Fifth ed., Oxford

Univ. Press, 1979.

(24)

[6] G. HARMAN, A. V. KUMCHEV, On sums of squares of primes. Math. Proc. Cambridge Philos.

Soc., to appear.

[7] D.R. HEATH-BROWN, Cubic forms in ten variables. Proc. London Math. Soc. 47 (1983),

225-257.

[8] D.R. HEATH-BROWN. D.I.TOLEV, Lagrange’s four squares theorem with one prime and three almost-prime variables. J. Reine Angew. Math. 558 (2003), 159-224.

[9] L.K. HUA, Some results in the additive prime number theory. Quart. J. Math. Oxford 9 (1938), 68-80.

[10] L.K. HUA, Introduction to number theory. Springer, 1982.

[11] L.K. HuA, Additive theory of prime numbers. American Mathematical Society, Providence, 1965.

[12] H. IWANIEC, Rosser’s sieve. Acta Arith. 36 (1980), 171-202.

[13] H. IWANIEC, A new form of the error term in the linear sieve. Acta Arith. 37 (1980),

307-320.

[14] H.D. KLOOSTERMAN, On the representation of numbers in the form ax2 + by2 + cz2 + dt2.

Acta Math. 49 (1926), 407-464.

[15] J. LIU, On Lagrange’s theorem with prime variables. Quart. J. Math. Oxford, 54 (2003),

453-462.

[16] J. LIU, M.-C. LIU, The exceptional set in the four prime squares problem. Illinois J. Math.

44 (2000), 272-293.

[17] J.LIU, T. D. WOOLEY. G. Yu, The quadratic Waring-Goldbach problem. J. Number Theory,

107 (2004), 298-321.

[18] V.A. PLAKSIN, An asymptotic formula for the number of solutions of a nonlinear equation for prime numbers. Math. USSR Izv. 18 (1982), 275-348.

[19] P. SHIELDS, Some applications of the sieve methods in number theory. Thesis, University of Wales 1979.

[20] D.I. TOLEV, Additive problems with prime numbers of special type. Acta Arith. 96, (2000),

53-88.

[21] D.I. TOLEV, Lagrange’s four squares theorem with variables of special type. Proceedings of

the Session in analytic number theory and Diophantine equations, Bonner Math. Schriften, Bonn, 360 (2003).

[22] T.D. WOOLEY, Slim exceptional sets for sums of four squares, Proc. London Math. Soc.

(3), 85 (2002), 1-21.

Doychin TOLEV

Department of Mathematics Plovdiv University "P. Hilendarski"

24 "Tsar Asen" str.

Plovdiv 4000, Bulgaria

E-mail : dtolev@pu.acad.bg

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